The emission region has a half flux radius of 0.05 au, which remains relatively constant between the center channels within the uncertainties. With Br\(\gamma \)  emission coming from a region similar in extent to the corotation radius, it is likely that magnetospheric accretion is a driving mechanism behind a large part of the total line emission and that a significant portion of the emission will originate in the accretion columns of the magnetosphere. At about 5.9 R\(_*\) , this size falls into the range of values typically associated with magnetospheres [1]}.
